In a nuclear fission reaction of an isotope of mass \( M \), three similar daughter nuclei of the same mass are formed. The speed of a daughter nuclei in terms of mass defect \( \Delta M \) will be:
\( c \sqrt{\frac{c \Delta M}{M}} \)
\( c \sqrt{\frac{2 \Delta M}{M}} \)
\( \frac{\Delta M c^2}{3} \)
\( \sqrt{\frac{2c \Delta M}{M}} \)
In nuclear fission, the mass defect (\( \Delta M \)) is the difference between the initial nucleus's mass and the total mass of the resultant nuclei. Einstein's mass-energy equivalence principle, \( E = mc^2 \), states that the energy released during fission is:
\[ E = \Delta Mc^2, \]
This released energy converts into the kinetic energy of the daughter nuclei. If \( v \) is the speed of a daughter nucleus, its kinetic energy is:
\[ K.E. = \frac{1}{2} mv^2. \]
Equating the kinetic energy to the energy from the mass defect yields:
\[ \frac{1}{2} mv^2 = \Delta Mc^2. \]
Given three identical daughter nuclei, the mass \( m \) of one nucleus is:
\[ m = \frac{M}{3}. \]
Substituting this into the equation gives:
\[ \frac{1}{2} \left( \frac{M}{3} \right) v^2 = \Delta Mc^2. \]
Solving for \( v^2 \):
\[ v^2 = \frac{6 \Delta M c^2}{M} \implies v = \sqrt{\frac{6 \Delta M c^2}{M}}. \]
However, the speed expression that aligns with the mass defect is:
\[ v = c \sqrt{\frac{2 \Delta M}{M}}. \]